The Cassegrain reflector is a folded optics design, using two mirrors to fold the light path back on itself. This increases the focal length of the telescope, without increasing it's length. By doing so you can compact a more powerful telescope into a smaller frame, which has advantages for small amateur scopes (portability) and large professional ones (reduced cost).
First developed in 1672 by Laurent Cassegrain, this reflector is a combination of a primary concave mirror and a secondary convex mirror, both aligned symmetrically about the optical axis. The primary mirror usually contains a hole in the centre thus permitting the light to reach an eyepiece, a camera, or a light detector. The primary mirror is parabolic while the secondary mirror is hyperbolic.
Of the three basic types of telescopes: refractors, reflectors and catadioptrics, the Cassegrain reflector falls under the categories of reflecting and Catadioptric designs.
Laurent Cassegrain, a French priest and astronomer, invented the Cassegrain telescope in the mid-17th century. The design features a concave primary mirror with a secondary convex mirror, allowing light to be reflected back through a hole in the primary mirror for viewing.
The Cassegrain has a hole in the mirror, at the bottom of the scope, where the reflector mirror reflects the light onto the viewing piece. So, the Cassegrain is a reflection telescope but it's primary and secondary mirrors work a bit differently than most reflecting telescopes.
A telescope design that has a hole in the center of the main mirror is called a "Cassegrain telescope." This design uses a secondary mirror to reflect the light back through the hole in the primary mirror to the eyepiece or sensor, allowing for a more compact design and longer focal length.
Reflecting telescopes use concave mirrors to gather and focus light to form an image. The primary mirror in a reflecting telescope collects incoming light and reflects it to a secondary mirror, which then directs the light to the eyepiece or camera for viewing. This design is commonly used in telescopes like Newtonian reflectors and Cassegrain telescopes.
The Telescope Inventor, Hans Lippershey, was believed to have been in his 40s when he made the telescope around 1608.
A Cassegrain reflector
The HST is a Cassegrain reflector telescope.
Cassegrain
HST's primary mirror is a Cassegrain Reflector.
Laurent Cassegrain, a French priest and astronomer, invented the Cassegrain telescope in the mid-17th century. The design features a concave primary mirror with a secondary convex mirror, allowing light to be reflected back through a hole in the primary mirror for viewing.
The Cassegrain has a hole in the mirror, at the bottom of the scope, where the reflector mirror reflects the light onto the viewing piece. So, the Cassegrain is a reflection telescope but it's primary and secondary mirrors work a bit differently than most reflecting telescopes.
The main differences between a Dobsonian telescope and a Schmidt-Cassegrain telescope are their design and portability. Dobsonian telescopes are simpler in design and offer larger apertures for better light-gathering ability, making them ideal for deep-sky observation. Schmidt-Cassegrain telescopes, on the other hand, are more compact and versatile, with a folded optical path that allows for a longer focal length in a shorter tube. They are better suited for planetary and lunar observation. For stargazing needs focused on deep-sky objects, a Dobsonian telescope would be more suitable due to its larger aperture and simpler design. If you are interested in planetary and lunar observation, a Schmidt-Cassegrain telescope may be a better choice for its compactness and versatility.
A telescope design that has a hole in the center of the main mirror is called a "Cassegrain telescope." This design uses a secondary mirror to reflect the light back through the hole in the primary mirror to the eyepiece or sensor, allowing for a more compact design and longer focal length.
It does not have a magnification properly speaking since it works as a camera, not a visual telescope. The aperture of the Cassegrain-Schmidt mirror is 2.4 m. The main camera has 16 MB.
Different telescopes utilize different parts of the electromagnetic spectrum. Two types of optical telescope are refracting and reflecting. There are also different kinds of radio telescope investigating different bandwidths from the infra red to the untra violet
No - HSTs' primary mirror is a Cassegrain Reflector of Ritchey-Chrétien design, which contains a hyperbolic primary/secondary mirror.
Mercury barometer - invented by Evangelist Torricelli (1608) barometer Aneroid barometer - invented by Lucien Vidie in 1843 Cassegrain telescope thermometer pendulum clock